Quantitative Spectral Classification. Analysis of K-M Giant Stars in the Visible and Near-IR region

Details Quantitative Spectral Classification. Analysis of K-M Giant Stars in the Visible and Near-IR region Quantitative Spectral Classification. Analysis of K-M Giant Stars in the Visible and Near-IR region

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..25..105m&link_type=abstract

Third International Meeting of Dynamic Astronomy in Latin America (Eds. Carlos Abad, Ángel Bongiovanni, & Yaneth Guillén) Revist

Astronomy and Astrophysics

Astronomy

Methods: Numerical, Stars: Fundamental Parameters

Scientific paper

The absolute magnitude M[V] and the color B-V are recovered for a set of
220 K-M stars through two independent ways: A function fitting which
involves linear polynomials and artificial neural networks (ANN). In
both cases, similar results are found.

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